Is there any way to calculate (or at least estimate) mass of an exoplanet from transit method? I know that mass can be calculated with radial velocity method, however I would like to create program for processing Kepler light curves (without radial velocity data).
The data I have are:
- radius, mass, surface temperature and luminosity of star,
- orbital period, semi-major axis and radius of exoplanet,
- duration and depth of transit.